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Question

Q.(a)

(i) A plane light wave propagating from a rarer into a denser medium is incident at an angle ii on the surface separating the two media. Using Huygens's principle, draw the refracted wave and hence verify Snell's law of refraction.
(ii) In a Young's double-slit experiment, the slits are separated by 0.30 mm and the screen is kept 1.5 m away. The wavelength of light used is 600 nm. Calculate the distance between the central bright fringe and the 4th dark fringe.
(OR)
(b)
(i) Discuss briefly the diffraction of light from a single slit and draw the shape of the diffraction pattern.
(ii) An object is placed between the pole and the focus of a concave mirror. Using the mirror formula, prove mathematically that it produces a virtual and enlarged image.
CBSECBSE Class XII Board 2024Subjective· 5mImportance★★★★★
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Figure — Part (a)(i) requires drawing the Huygens refracted wavefront to verify Snell's law; the catalog figure shows e
Figure — Part (a)(i) requires drawing the Huygens refracted wavefront to verify Snell's law; the catalog figure shows e

Part (a): Huygens's construction gives Snell's law sin⁡isin⁡r=v1v2=n21\dfrac{\sin i}{\sin r}=\dfrac{v_1}{v_2}=n_{21}; the 4th dark fringe lies y4=1.05 cmy_4=1.05\,\text{cm} from the centre. Part (b): single-slit diffraction gives a broad central maximum with minima at asin⁡θ=mλa\sin\theta=m\lambda; for a concave mirror an object between pole and focus forms a virtual, erect, enlarged image.

Part (a)

(i) Snell's law from Huygens's principle

Every point on a wavefront is a source of secondary spherical wavelets; the new wavefront is their envelope. Let plane wavefront ABAB be incident at angle ii on the surface between a rarer medium (speed v1v_1) and a denser medium (speed v2<v1v_2<v_1). Suppose AA reaches the surface at t=0t=0 and BB reaches the surface at B′B' after time tt, travelling BB′=v1tBB'=v_1 t in medium 1. In the same time the wavelet from AA advances v2tv_2 t into medium 2. Drawing an arc of radius v2tv_2 t about AA and the tangent from B′B' gives the refracted wavefront A′B′A'B', making angle rr with the surface.

In the right triangles on the common line AB′AB':

sin⁡i=BB′AB′=v1tAB′,sin⁡r=AA′AB′=v2tAB′.\sin i=\frac{BB'}{AB'}=\frac{v_1 t}{AB'},\qquad \sin r=\frac{AA'}{AB'}=\frac{v_2 t}{AB'}.

Dividing,

sin⁡isin⁡r=v1v2=c/v2c/v1=n2n1=n21.\frac{\sin i}{\sin r}=\frac{v_1}{v_2}=\frac{c/v_2}{c/v_1}=\frac{n_2}{n_1}=n_{21}.

This is Snell's law.

Watch out

Going from a rarer to a denser medium the ray bends toward the normal (r<ir<i).

(ii) Position of the 4th dark fringe

Given d=0.30 mm=3.0×10−4 md=0.30\,\text{mm}=3.0\times10^{-4}\,\text{m}, D=1.5 mD=1.5\,\text{m}, λ=600 nm=6.0×10−7 m\lambda=600\,\text{nm}=6.0\times10^{-7}\,\text{m}. Dark fringes require path difference (2n−1)λ/2(2n-1)\lambda/2, so

yn=(2n−1)λD2d.y_n=\frac{(2n-1)\lambda D}{2d}.

For the 4th dark fringe, n=4n=4: …

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